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Ultra high energy cosmic rays

Nuclear Physics B - Proceedings Supplements, 2001
Abstract The evidence for the existence of cosmic rays with energies in excess of 1020 eV is now overwhelming. There is so far no indication of the GZK cutoff in the energy spectrum at 5 × 1019 eV. This conclusion is not firm for lack of statistics. A cutoff would be expected if the sources of the cosmic rays were distributed uniformly throughout the
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Ultra high energy cosmic rays

Contemporary Physics, 2010
Ultra High Energy Cosmic Rays (UHECRs) represent the most energetic source of elementary particles available to scientists. They have macroscopic energies, exceeding 5 × 1019 eV, and as yet unidentified sources. Unfortunately, their flux is as low as one particle per century per square kilometre, requiring dedicated detectors with huge apertures to ...
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Ultra High Energy Cosmic Rays

1983
The interpretation of observations on cosmic rays above 1015 eV is discussed in simple terms, without considering detailed models. The variation of the amplitude of anisotropy with energy (compared with a “leaky box” picture) and the anisotropy in galactic latitude (indicating a local density gradient) strongly suggest a galactic origin for particles ...
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Are gamma-ray bursts the sources of ultra-high energy cosmic rays?

Astroparticle Physics, 2015
Philipp Baerwald   +2 more
exaly  

Cosmogenic photons as a test of ultra-high energy cosmic ray composition

Astroparticle Physics, 2011
Dan Hooper, Andrew M Taylor, S Sarkar
exaly  

Optimized trigger for ultra-high-energy cosmic-ray and neutrino observations with the low frequency radio array

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2012
M Mevius, O Scholten, A Van Ardenne
exaly  

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